5XMM J124621.9+022839
5XMM-DR15 stacked source · SRCID 3005176010100056
Position:
12h46m21.95s +02d28m39.6s
(191.59148°, 2.47765°)
EP flux
6.37e-15
± 2.1e-15
erg cm-2 s-1
CLASSX
AGN
(0.677)
Detections
8
| SRCID | 3005176010100056 |
|---|---|
| IAUNAME | 5XMM J124621.9+022839 |
| SC_RA | 12h46m21.95s (191.59148°) |
| SC_DEC | +02d28m39.6s (2.47765°) |
| RADEC_ERR | 0.84 arcsec |
| LII / BII | 299.8969° / 65.3195° |
| N_CONTRIB | 8 (detections) |
| N_OBS | 8 (observations covering the position) |
| MJD_FIRST | 52077.875 (2001-06-17 20:59:59.000 UTC) |
| MJD_LAST | 57038.758 (2015-01-16 18:11:59.000 UTC) |
Stacked EPIC flux
EP flux (0.2-12 keV): 6.37e-15 ± 2.1e-15 erg cm-2 s-1
Hardness ratios
HR1
0.80
± 0.16
0.2-0.5 / 0.5-1.0 keV
HR2
0.15
± 0.12
0.5-1.0 / 1.0-2.0 keV
HR3
-0.16
± 0.12
1.0-2.0 / 2.0-4.5 keV
HR4
-0.64
± 0.27
2.0-4.5 / 4.5-12.0 keV
Extent:
0.00
arcsec
(ML -0.2)
SUM_FLAG:
1
Long-term lightcurve
No light-curve points available.
AGN
CLASSX outlier: 2.38
Class probabilities
Class taxonomy
- AGN — active galactic nucleus.
- Bkg_AGN — background AGN.
- Star — Galactic star.
- Gal_XRB — Galactic X-ray binary.
- Extragal_XRB — extragalactic X-ray binary.
- CV — cataclysmic variable.
- Extended — cluster or galaxy.
Optical Monitor (OM)
- OM Source ID
- 3282730
- Match probability
- 0.62
| Filter | Mag (AB) | Err |
|---|---|---|
| UVW2 | — | — |
| UVM2 | — | — |
| UVW1 | — | — |
| U | 22.206 | 0.220 |
| B | — | — |
| V | — | — |
CLASSOPT
- Class
- Star
Star
AGN
Galaxy
No redshift estimate available for this source.
Stacked power-law fit
| Unabsorbed flux | 8.18e-15 (+1.2e-14 / −5.6e-15) erg cm−2 s−1 |
|---|---|
| NH | 5.95e+20 (+2.8e+21 / −3.9e+19) cm−2 |
| Photon index (Γ) | 1.74 (+2.39 / −1.30) |
| DoF | 68 |
| p-value | 0.609 |
| Quality flag | 0 |
No variability data available for this source.
No contributing observations found.
Sky view (optical)
DSS2 colour optical image. The header thumbnail shows the XMM-Newton X-ray image; use the layers menu in the toolbar to switch surveys.
Hardness-ratio diagram
No hardness-ratio pairs available for this source.
The per-observation light curve is shown in the X-ray properties section above.